ALMA Memo 585 Loss of Gold Plated Waveguides at 210-280 GHz

نویسنده

  • A. R. Kerr
چکیده

The loss at 210-280 GHz of room temperature waveguides plated with BDT 200 bright gold and Pur-A-Gold 125 soft gold is within ~10% of the theoretical loss based on the DC conductivity of pure gold and the classical skin effect. This is not the case for some other types of gold plating meeting the same ASTM (or MIL) specs but in which a trace of nickel is used as a brightener. Introduction Following the recent replacement of the NRAOCDL bright-gold plating solution used for the ALMA Band 6 SIS mixers, it was noticed that an initial darkening of the surface occurred on immersion of the brass parts in the bath. Although the final plating had good adhesion and appeared to be of high quality, we were disconcerted by the change in behavior of the bath and decided to measure the microwave loss of plated waveguide samples. Our concern was that the manufacturer might have made a subtle change in the composition of the solution which would not affect its ASTM specification but could increase the microwave loss. Recently, we had observed that the nickel brightener used in some commercial gold plating baths could cause significantly increased microwave loss, even though the plating met the appropriate ASTM (or MIL) specs. Plating Processes The NRAO-CDL plating lab uses two gold plating processes, one for hard, bright, gold based on the Enthone BDT 200 bath [1] which uses an arsenic brightener, and the other for soft, wirebondable gold based on the Enthone Pur-A-Gold 125 bath [1]. According to the manufacturer's data sheets, BDT 200 meets ASTM B 488-01 Type I (purity > 99.7%) Code C (hardness 130-200 KH25), while Pur-A-Gold 125 meets ASTM B 488-01 Type III (purity > 99.9% Code A (hardness # 90 KH25). The test waveguides were plated with 75 μ-in of gold, which is about ten skin depths in the frequency band of measurement. Fig. 1. The waveguide pattern in the test pieces. The waveguide is WR-3.7 (0.037" x 0.0185"). The total waveguide length is 10.000 inches.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ALMA MEMO NO. 412 68.5 to 118 GHz Measurements of Possible Infrared Filter Materials: Black Polyethylene, Zitex, and Grooved and Un-Grooved Fluorogold and HDPE

For the ALMA production test receivers at present being designed in the NRAO CDL, there is a need for infrared filters to reduce the thermal loading. One possibility is to use a plastic material which has reasonable absorption or scattering for the infrared wavelengths but low loss at the signal wavelengths. Black polyethylene (polyethylene with carbon filler) [1, 2], Zitex (expanded PTFE) [3],...

متن کامل

ALMA Memo 381 Elements for E-Plane Split-Block Waveguide Circuits

E-plane split-block waveguide construction is well suited to many millimeter-wave components, including power dividers, frequency multipliers, and single-ended, balanced and sideband-separating mixers [1]. Recent ALMA memos have described quadrature hybrids [2] and a matched power divider [3] suitable for split-block construction. This memo describes four additional waveguide elements which can...

متن کامل

The Dual - Load Calibration device revisited

Following ALMA memo 371, I re-investigate the dual load calibration scheme which has been proposed for ALMA. This memo improves on the requirements derived in memo 371 by using a better prediction for the atmospheric fluctuations at short time scales. It is shown that because of atmospheric properties and of the antenna geometry, a dual-load system located in the ALMA antenna subreflectors need...

متن کامل

ALMA Memo #303 Water Vapour Radiometers for ALMA

The JCMT-CSO single-baseline interferometer was the first to demonstrate phase correction using the 183 GHz line, using equipment built by Martina Wiedner, Richard Hills and colleagues. Only a limited quantity of data were gathered but the results (ALMA memo 252) were encouraging and suggested that even an uncooled system could provide effective phase calibration at submillimetre wavelengths. S...

متن کامل

ALMA memo 435 A Hybrid Option for the First LOs using Direct Photonic LO Driver

We propose a hybrid option for the first local oscillators (LOs) of ALMA in which a direct photonic LO driver is used to drive cold multipliers. The photomixer using NTT uni-travelling carrier photodiode has been demonstrated to have high power of 2 m W at 100 GHz and low amplitude noise of < 7 − 17 K/μW in the frequency range of 98 − 105 GHz. This option simplifies the LO part of the cartridge...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009